The Johns Hopkins Gazette: January 6, 2003
January 6, 2003
VOL. 32, NO. 16


Volcanoes on Jupiter's Moon Io Spew Salt Into Atmosphere

Astronomers' recent discovery solves a nearly 30-year-old mystery

By Michael Purdy

Johns Hopkins Gazette Online Edition

Astronomers at Johns Hopkins, the Observatoire de Paris and other institutions have solved a nearly 30-year-old mystery surrounding Jupiter's moon Io, showing that volcanoes there appear to be shooting gaseous salt into the moon's thin atmosphere.

Further analysis of the results, including modeling how the salt is broken down into sodium and chlorine atoms, could help planetary scientists move closer to determining what kinds of meteoritic materials originally came together to form Io, according to Darrell Strobel, professor of Earth and Planetary Sciences in the Krieger School of Arts and Sciences.

Strobel was an author of a paper on the new results published in Nature on Jan. 2. He said the finding brought closure to a study in 1974 that revealed neutral clouds of sodium around Io. That finding was made by Bob Brown, an astronomer who at the time was doing postdoctoral work at Harvard.

"He told me some years afterwards, 'This discovery of mine is so simple, I was amazed somebody hadn't done it 30 to 40 years earlier,' " said Strobel. "Nobody was looking for it, nobody would have guessed it was there."

Astronomers winnowed the list of theoretical suspects for the source of sodium for years before determining the most likely suspect was salt, or sodium chloride. That conclusion was reached after the detection two years ago of chlorine in a doughnut-shaped, electrically charged cloud of gas around Io known as the plasma torus. Based on the new chlorine finding and the theoretical work, astronomers decided to conduct the exacting studies necessary to look for salt.

"The bottom line is that there seems to be enough salt in Io's volcanic atmosphere to supply both the amount of sodium that one sees in the neutral clouds and the chlorine in the plasma torus," said Strobel, who is also a professor of physics and astronomy at Johns Hopkins.

A slightly eccentric orbit around Jupiter and the gravitational fields of two nearby large moons, Europa and Ganymede, subject Io to a great deal of stress, flexing the moon's crust and heating its core. As a result, Io, which is roughly comparable in size to Earth's moon, is hands-down the most volcanically active planetary body in the solar system. Io's frequently active volcanoes would make it a hell for anyone who might want to visit, but it's a heaven for scientists eager to watch a planetary body regularly belch up tons of its innards.

"Roughly two tons of volcanic material are tossed into Io's magnetosphere every second, and then when this material is ionized [electrically charged], the inner magnetosphere starts to resemble a miniature pulsar," Strobel said.

Interactions between the clouds of electrically charged gas around Io and electrically charged particles in Jupiter's polar atmosphere speed up the rotation of the charged particles around Io but also apply an infinitesmal drag to the rotation of Jupiter, gradually slowing the speed at which the giant planet spins.

"It's a remarkable, unique system of interaction," Strobel said. "We've learned quite a bit since the days when Voyager 1 first swept by the moon in 1979 and revealed eight active volcanoes, but we don't understand it completely."

Strobel said the lead author of the new Nature paper, Emmanuel Lellouch of the Observatoire de Paris, had looked previously for salt in Io's atmosphere and failed to find signs of it. Co-author Nicholas Snyder of the University of Colorado at Boulder, one of the researchers who discovered chlorine in Io's plasma torus, suggested using the millimeter-wavelength radio telescope at the Institut de Radio-Astronomie Millimetrique in Granada, Spain, to perform a definitive search for salt.

Observations with a millimeter-wavelength radio telescope force astronomers to focus on very tiny regions of the spectrum, making it necessary to carefully choose the frequencies they want to observe. But when the team conducted its studies in January 2002, they found the characteristic spectroscopic lines they were looking for. An examination of potential sources for the salt in the atmosphere pointed to the volcanoes as the most likely point of origin for the salt.

Other authors on the paper were Gabriel Paubert of the Institut de Radio-Astronomie Millimetrique and Julianne Moses of NASA's Lunar and Planetary Institute. This research was supported by the NASA Planetary Atmospheres Program.